The Solar System: A New Geometric Classification and Prediction of a New Asteroid

Ahmad Hazaymeh; Mosab Hawarey; Khaled Hazaymeh

doi:doi:10.11648/j.ijass.20150302.11

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The Solar System: A New Geometric Classification and Prediction of a New Asteroid

Ahmad Hazaymeh, Mosab Hawarey, Khaled Hazaymeh

Published in International Journal of Astrophysics and Space Science (Volume 3, Issue 2)

Received: 21 December 2013 Accepted: 13 March 2015 Published: 24 March 2015

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Abstract

One of the most popular theories of measuring planetary distances in the solar system is Bode's law, but this law has some deviations when compared to the real distances. In this paper a new classification (Hazaymeh-Hawarey Classification) is presented. This classification aims to explain the inability of Bode's law to identify the two orbital dimensions of Neptune and Pluto, and it provides a new geometric image for the orbital distribution of the solar system, including Neptune and Pluto. This new classification shows that orbits of the solar system are divided into four equal groups, where the (10/3 = 4) is true. It also discovers that the two dimensions of Neptune and Pluto are much more systematic in the solar system, compared to Bode's law. The new classification includes the adjustment of the distances of Sedna and Eris, and enables the mathematical identification of a new asteroid located after Iris, even before the astronomical verification. The new classification reveals the symmetry and the anomaly of the solar system orbits and that the diameters of the first and fourth groups follow a geometric sequence. According to this, the diameter of the new asteroid can be determined.

Published in	International Journal of Astrophysics and Space Science (Volume 3, Issue 2)
DOI	10.11648/j.ijass.20150302.11
Page(s)	16-19
Creative Commons	This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.
Copyright	Copyright © The Author(s), 2024. Published by Science Publishing Group

Keywords

Bode's Law, Orbital Distances, New Geometry of the Solar System, New Astroid

References

[1]	Nieto, M. (1972) The Titius-Bode law of planetary distances: its history and theory, 1st ed. Oxford, UK: Pergamon Press.
[2]	Graner, F. & Dubrulle, B. (1994) Titius-Bode laws in the solar system I. Scale invariance explains everything. Astronomy & Astrophysics, Vol. 282, No. 1, pp. 262-268.
[3]	Hayes, W. & Tremaine, S. (1998) Fitting selected random planetary systems to Titius-Bode laws. Icarus, Vol. 135, No. 2, pp. 549-557. DOI: 10.1006/icar.1998.5999.
[4]	Lynch, P. (2003) On the significance of the Titius–Bode law for the distribution of the planets. Monthly Notice of the Royal Astronomical Society, Vol. 341, No. 4, pp. 1174–1178. DOI: 10.1046/j.1365-8711.2003.06492.x.
[5]	Brown, M., Trujillo, C. & Rabinowitz, D. (2004) Discovery of a Candidate Inner Oort Cloud Planetoid. Astrophysical Journal, Vol. 617, No. 1, pp. 645–649. DOI: 10.1086/422095.
[6]	Stansberry, J., Grundy, W., Brown, M., Cruikshank, D., Spencer, J., Trilling, D. & Margot, J.-L. (2007) 'Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope' In: Barucci, M. A., Boehnhardt, H. & Cruikshank, D. P. (eds.) The Solar System Beyond Neptune. University of Arizona Press, pp. 161–179.

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APA Style

Ahmad Hazaymeh, Mosab Hawarey, Khaled Hazaymeh. (2015). The Solar System: A New Geometric Classification and Prediction of a New Asteroid. International Journal of Astrophysics and Space Science, 3(2), 16-19. https://doi.org/10.11648/j.ijass.20150302.11

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ACS Style

Ahmad Hazaymeh; Mosab Hawarey; Khaled Hazaymeh. The Solar System: A New Geometric Classification and Prediction of a New Asteroid. Int. J. Astrophys. Space Sci. 2015, 3(2), 16-19. doi: 10.11648/j.ijass.20150302.11

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AMA Style

Ahmad Hazaymeh, Mosab Hawarey, Khaled Hazaymeh. The Solar System: A New Geometric Classification and Prediction of a New Asteroid. Int J Astrophys Space Sci. 2015;3(2):16-19. doi: 10.11648/j.ijass.20150302.11

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@article{10.11648/j.ijass.20150302.11,
  author = {Ahmad Hazaymeh and Mosab Hawarey and Khaled Hazaymeh},
  title = {The Solar System: A New Geometric Classification and Prediction of a New Asteroid},
  journal = {International Journal of Astrophysics and Space Science},
  volume = {3},
  number = {2},
  pages = {16-19},
  doi = {10.11648/j.ijass.20150302.11},
  url = {https://doi.org/10.11648/j.ijass.20150302.11},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijass.20150302.11},
  abstract = {One of the most popular theories of measuring planetary distances in the solar system is Bode's law, but this law has some deviations when compared to the real distances. In this paper a new classification (Hazaymeh-Hawarey Classification) is presented. This classification aims to explain the inability of Bode's law to identify the two orbital dimensions of Neptune and Pluto, and it provides a new geometric image for the orbital distribution of the solar system, including Neptune and Pluto. This new classification shows that orbits of the solar system are divided into four equal groups, where the (10/3 = 4) is true. It also discovers that the two dimensions of Neptune and Pluto are much more systematic in the solar system, compared to Bode's law. The new classification includes the adjustment of the distances of Sedna and Eris, and enables the mathematical identification of a new asteroid located after Iris, even before the astronomical verification. The new classification reveals the symmetry and the anomaly of the solar system orbits and that the diameters of the first and fourth groups follow a geometric sequence. According to this, the diameter of the new asteroid can be determined.},
 year = {2015}
}

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TY  - JOUR
T1  - The Solar System: A New Geometric Classification and Prediction of a New Asteroid
AU  - Ahmad Hazaymeh
AU  - Mosab Hawarey
AU  - Khaled Hazaymeh
Y1  - 2015/03/24
PY  - 2015
N1  - https://doi.org/10.11648/j.ijass.20150302.11
DO  - 10.11648/j.ijass.20150302.11
T2  - International Journal of Astrophysics and Space Science
JF  - International Journal of Astrophysics and Space Science
JO  - International Journal of Astrophysics and Space Science
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PB  - Science Publishing Group
SN  - 2376-7022
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AB  - One of the most popular theories of measuring planetary distances in the solar system is Bode's law, but this law has some deviations when compared to the real distances. In this paper a new classification (Hazaymeh-Hawarey Classification) is presented. This classification aims to explain the inability of Bode's law to identify the two orbital dimensions of Neptune and Pluto, and it provides a new geometric image for the orbital distribution of the solar system, including Neptune and Pluto. This new classification shows that orbits of the solar system are divided into four equal groups, where the (10/3 = 4) is true. It also discovers that the two dimensions of Neptune and Pluto are much more systematic in the solar system, compared to Bode's law. The new classification includes the adjustment of the distances of Sedna and Eris, and enables the mathematical identification of a new asteroid located after Iris, even before the astronomical verification. The new classification reveals the symmetry and the anomaly of the solar system orbits and that the diameters of the first and fourth groups follow a geometric sequence. According to this, the diameter of the new asteroid can be determined.
VL  - 3
IS  - 2
ER  -

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Author Information

Ahmad Hazaymeh

Geodesic Dome Company, Astronomy and Mathematics Division, New York, NY 10001, USA
Mosab Hawarey

Geodesic Dome Company, Geodesy and Geophysics Division, New York, NY 10001, USA
Khaled Hazaymeh

University of Calgary, Department of Geomatics Engineering, Calgary, Alberta, Canada

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Plain Text BibTeX RIS

APA Style

Ahmad Hazaymeh, Mosab Hawarey, Khaled Hazaymeh. (2015). The Solar System: A New Geometric Classification and Prediction of a New Asteroid. International Journal of Astrophysics and Space Science, 3(2), 16-19. https://doi.org/10.11648/j.ijass.20150302.11

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ACS Style

Ahmad Hazaymeh; Mosab Hawarey; Khaled Hazaymeh. The Solar System: A New Geometric Classification and Prediction of a New Asteroid. Int. J. Astrophys. Space Sci. 2015, 3(2), 16-19. doi: 10.11648/j.ijass.20150302.11

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AMA Style

Ahmad Hazaymeh, Mosab Hawarey, Khaled Hazaymeh. The Solar System: A New Geometric Classification and Prediction of a New Asteroid. Int J Astrophys Space Sci. 2015;3(2):16-19. doi: 10.11648/j.ijass.20150302.11

Copy | Download

@article{10.11648/j.ijass.20150302.11,
  author = {Ahmad Hazaymeh and Mosab Hawarey and Khaled Hazaymeh},
  title = {The Solar System: A New Geometric Classification and Prediction of a New Asteroid},
  journal = {International Journal of Astrophysics and Space Science},
  volume = {3},
  number = {2},
  pages = {16-19},
  doi = {10.11648/j.ijass.20150302.11},
  url = {https://doi.org/10.11648/j.ijass.20150302.11},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijass.20150302.11},
  abstract = {One of the most popular theories of measuring planetary distances in the solar system is Bode's law, but this law has some deviations when compared to the real distances. In this paper a new classification (Hazaymeh-Hawarey Classification) is presented. This classification aims to explain the inability of Bode's law to identify the two orbital dimensions of Neptune and Pluto, and it provides a new geometric image for the orbital distribution of the solar system, including Neptune and Pluto. This new classification shows that orbits of the solar system are divided into four equal groups, where the (10/3 = 4) is true. It also discovers that the two dimensions of Neptune and Pluto are much more systematic in the solar system, compared to Bode's law. The new classification includes the adjustment of the distances of Sedna and Eris, and enables the mathematical identification of a new asteroid located after Iris, even before the astronomical verification. The new classification reveals the symmetry and the anomaly of the solar system orbits and that the diameters of the first and fourth groups follow a geometric sequence. According to this, the diameter of the new asteroid can be determined.},
 year = {2015}
}

Copy | Download

TY  - JOUR
T1  - The Solar System: A New Geometric Classification and Prediction of a New Asteroid
AU  - Ahmad Hazaymeh
AU  - Mosab Hawarey
AU  - Khaled Hazaymeh
Y1  - 2015/03/24
PY  - 2015
N1  - https://doi.org/10.11648/j.ijass.20150302.11
DO  - 10.11648/j.ijass.20150302.11
T2  - International Journal of Astrophysics and Space Science
JF  - International Journal of Astrophysics and Space Science
JO  - International Journal of Astrophysics and Space Science
SP  - 16
EP  - 19
PB  - Science Publishing Group
SN  - 2376-7022
UR  - https://doi.org/10.11648/j.ijass.20150302.11
AB  - One of the most popular theories of measuring planetary distances in the solar system is Bode's law, but this law has some deviations when compared to the real distances. In this paper a new classification (Hazaymeh-Hawarey Classification) is presented. This classification aims to explain the inability of Bode's law to identify the two orbital dimensions of Neptune and Pluto, and it provides a new geometric image for the orbital distribution of the solar system, including Neptune and Pluto. This new classification shows that orbits of the solar system are divided into four equal groups, where the (10/3 = 4) is true. It also discovers that the two dimensions of Neptune and Pluto are much more systematic in the solar system, compared to Bode's law. The new classification includes the adjustment of the distances of Sedna and Eris, and enables the mathematical identification of a new asteroid located after Iris, even before the astronomical verification. The new classification reveals the symmetry and the anomaly of the solar system orbits and that the diameters of the first and fourth groups follow a geometric sequence. According to this, the diameter of the new asteroid can be determined.
VL  - 3
IS  - 2
ER  -

Copy | Download